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astro-ph2002★ 1 cited
Can Hydrostatic Cores Form Within Isothermal Molecular Clouds?
Enrique Vazquez-Semadeni, Mohsen Shadmehri, Javier Ballesteros-Paredes
Under the assumptions that molecular clouds are nearly spatially and temporally isothermal and that the density peaks (``cores'') within them are formed by turbulent fluctuations,…
astro-ph1999
Turbulent dissipation in the interstellar medium: implications for galaxy formation and evolution
V. Avila-Reese, E. Vázquez-Semadeni
We study turbulent dissipation in the ISM and explore some implications for galaxy formation and evolution using 2D MHD numerical simulations of compressible fluids. The turbulent…